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Star · A6IV

HIP 43338

HIP 43338 is a subgiant star of spectral type A6IV in the constellation Pyxis, 281.2 light-years from the Sun.

ConstellationPyxis
Distance281.2 light-years (86.2 pc)
Apparent magnitudemagnitude 6.48
Absolute magnitudemagnitude 1.80
Spectral typeA6IV
Surface temperature7,750 K
Luminosity16.8 L☉
Radius2.27 R☉
Mass2.03 M☉ (estimated)
Right ascension (J2000)8h 49m 44.9s
Declination (J2000)−21° 02′ 54″
Space velocity (relative to the Sun)23.6 km/s

In the sky

Visible to the naked eye under a dark sky (apparent magnitude 6.48). Visible from the whole Southern Hemisphere and north to latitude 69° N. South of latitude 69° S it never sets. It stands highest at midnight in January, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1745. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 5.0 million years.

The Sun seen from there

From a planet around HIP 43338, the Sun would look like a star of magnitude 9.51, in the direction where our sky has the constellation Vulpecula. It would be invisible to the naked eye.

Neighbours

Its nearest neighbours in the catalogue (within 20 light-years):

  • HIP 43626 6.83 light-years
  • HIP 44483 17.4 light-years
  • HIP 42928 19.4 light-years

Open in the simulation

Position, brightness and colour from the HYG / AT-HYG catalogue; temperature, luminosity, radius and mass are approximate values computed from these observations.